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Title: | The 31 Deg2 Release of the Stripe 82 X-Ray Survey: The Point Source Catalog | Authors: | LaMassa, Stephanie M. Urry, C. Megan CAPPELLUTI, Nico Böhringer, Hans COMASTRI, Andrea Glikman, Eilat Richards, Gordon Ananna, Tonima Brusa, Marcella Cardamone, Carie Chon, Gayoung Civano, Francesca Farrah, Duncan Gilfanov, Marat Green, Paul Komossa, S. Lira, Paulina Makler, Martin MARCHESI, STEFANO Pecoraro, Robert Ranalli, Piero Salvato, Mara Schawinski, Kevin Stern, Daniel Treister, Ezequiel Viero, Marco |
Issue Date: | 2016 | Journal: | THE ASTROPHYSICAL JOURNAL | Number: | 817 | Issue: | 2 | First Page: | 172 | Abstract: | We release the next installment of the Stripe 82 X-ray survey point-source catalog, which currently covers 31.3 deg<SUP>2</SUP> of the Sloan Digital Sky Survey (SDSS) Stripe 82 Legacy field. In total, 6181 unique X-ray sources are significantly detected with XMM-Newton (>5σ) and Chandra (>4.5σ). This catalog release includes data from XMM-Newton cycle AO 13, which approximately doubled the Stripe 82X survey area. The flux limits of the Stripe 82X survey are 8.7 × 10<SUP>-16</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, 4.7 × 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, and 2.1 × 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP> in the soft (0.5-2 keV), hard (2-10 keV), and full bands (0.5-10 keV), respectively, with approximate half-area survey flux limits of 5.4 × 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, 2.9 × 10<SUP>-14</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, and 1.7 × 10<SUP>-14</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>. We matched the X-ray source lists to available multi-wavelength catalogs, including updated matches to the previous release of the Stripe 82X survey; 88% of the sample is matched to a multi-wavelength counterpart. Due to the wide area of Stripe 82X and rich ancillary multi-wavelength data, including coadded SDSS photometry, mid-infrared WISE coverage, near-infrared coverage from UKIDSS and VISTA Hemisphere Survey, ultraviolet coverage from GALEX, radio coverage from FIRST, and far-infrared coverage from Herschel, as well as existing ∼30% optical spectroscopic completeness, we are beginning to uncover rare objects, such as obscured high-luminosity active galactic nuclei at high-redshift. The Stripe 82X point source catalog is a valuable data set for constraining how this population grows and evolves, as well as for studying how they interact with the galaxies in which they live. | URI: | http://hdl.handle.net/20.500.12386/24897 | URL: | https://iopscience.iop.org/article/10.3847/0004-637X/817/2/172 https://iopscience.iop.org/article/10.3847/0004-637X/817/2/172/pdf |
ISSN: | 0004-637X | DOI: | 10.3847/0004-637X/817/2/172 | Bibcode ADS: | 2016ApJ...817..172L | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1510.00852.pdf | preprint | 3.78 MB | Adobe PDF | View/Open |
LaMassa_2016_ApJ_817_172.pdf | pdf editoriale | 1.91 MB | Adobe PDF | View/Open |
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